tomoscan.esrf.scan.nxtomoscan.HDF5TomoScan#
- class tomoscan.esrf.scan.nxtomoscan.HDF5TomoScan(scan, entry=None, index=0, ignore_projections=None, nx_version=None)#
Bases:
NXtomoScan- __init__(scan, entry=None, index=0, ignore_projections=None, nx_version=None)#
Methods
__init__(scan[, entry, index, ...])build icat metadata dictionary filling NXtomo definition following icat definition: https://gitlab.esrf.fr/icat/hdf5-master-config/-/blob/88a975039694d5dba60e240b7bf46c22d34065a0/hdf5_cfg.xml
clear caches.
clear_caches()- rtype:
None
clear_frames_cache()clear_frames_caches()- rtype:
None
compute_reduced_darks([reduced_method, ...])- param ReduceMethod method:
method to compute the flats
compute_reduced_flats([reduced_method, ...])- param ReduceMethod method:
method to compute the flats
equal(other)- param instance to compare with :rtype:
bool:return: True if instance are equivalent
flat_field_correction(projs, proj_indexes[, ...])Apply flat field correction on the given data
from_dict(_dict)from_identifier(identifier)Return the Dataset from a identifier
get_bliss_orginal_files()- rtype:
str | None
get_bliss_original_files()- rtype:
str | None
get_bounding_box([axis])Return the bounding box covered by the Tomo object axis is expected to be in (0, 1, 2) or (x==0, y==1, z==2)
get_dark_expected_location()get_dataset_basename()- rtype:
str
get_detector_data_path()- rtype:
str
get_detector_transformations(default)get_distance(*args, **kwargs)get_energy_expected_location()get_flat_expected_location()return the dataset identifier of the scan.
get_ignored_projection_indices()get_master_file(scan_path)get_pixel_size([unit])- rtype:
float | None
get_pixel_size_expected_location()return a dictionary of all the projection.
get_projection_expected_location()return intensity monitor values for projections
get_relative_file(file_name[, ...])- type file_name:
str
get_sample_detector_distance([unit])- param unit:
unit requested for the distance
get_sample_detector_distance_expected_location()get_sinogram(line[, subsampling, norm_method])extract the sinogram from projections
get_valid_entries(file_path)return the list of 'Nxtomo' entries at the root level
get_volume_output_file_name([z, suffix])if used by tomwer and nabu this should help for tomwer to find out the output files of anbu from a configuration file.
get_x_flipped([default])get_y_flipped([default])is_abort(**kwargs)- return:
True if the acquisition has been abort
is_tomoscan_dir(directory, **kwargs)Check if the given directory is holding an acquisition
load_from_dict(_dict)Load properties contained in the dictionary.
load_reduced_darks([inputs_urls, ...])load reduced dark (median / mean...) into files
load_reduced_flats([inputs_urls, ...])load reduced flats frames
map_urls_on_scan_range(urls, n_projection, ...)map given urls to an angle regarding scan_range and number of projection.
node_is_nxtomo(node)check if the given h5py node is an nxtomo node or not
save_reduced_darks(darks[, output_urls, ...])Dump computed dark (median / mean...) into files.
save_reduced_flats(flats[, output_urls, ...])Dump computed dark (median / mean...) into files.
set_check_behavior([run_check, raise_error, ...])when user require to access to scan frames NXtomoScan build them (frames property).
set_reduced_darks(darks[, darks_infos])set_reduced_flats(flats[, flats_infos])to_dict()- rtype:
dict
update()Parse the root folder and files to update information
Attributes
DICT_PATH_KEYDICT_TYPE_KEYREDUCED_DARKS_DATAURLSREDUCED_DARKS_METADATAURLSREDUCED_FLATS_DATAURLSREDUCED_FLATS_METADATAURLSSCHEMEdict of projections made for alignment with acquisition index as key None if not found
count_time- rtype:
list | None
dark_n- rtype:
int | None
list of darks files
return tuple of Transformation affecting the NXdetector
dim_1- rtype:
int | None
dim_2- rtype:
int | None
distance- rtype:
float | None
Return the sample name
end_timeenergy in keV
entry- rtype:
str
estimated_cor_frm_motorexposure_time- rtype:
list | None
ff_interval- return:
field of view of the scan. None if unknown else Full or Half
number of flat per series (computed on the first series)
list of flats files
return tuple of frames.
if found dict of projections urls with index during acquisition as key
ignore_projectionsimage_key- rtype:
list | None
image_key_control- rtype:
list | None
- rtype:
str | None
intensity_monitorintensity_normalizationnumber of projection WITHOUT the return projections
nexus_pathnexus_version- rtype:
str | None
return x pixel size in meter
if found dict of projections urls with index during acquisition as key
Return a compacted view of projection frames.
reduced_darksreduced_darks_infosreduced_flatsreduced_flats_infosreturn_projs- rtype:
list | None
rotation_angle- rtype:
tuple | None
return sample detector distance in meter
if found dict of projections urls with index during acquisition as key
scan_range- rtype:
int | None
Return the sequence name
sourcesource_name- rtype:
float | None
source_typesplitted_flat_seriesplit flat according to flat indices
start_timetitlenumber of projection WITHOUT the return projections
- rtype:
str
warning: deprecated !!!!! return True if the frames are flip through x
return x pixel size in meter
x_real_pixel_size- rtype:
float | None
- return:
Estimated center of rotation estimated from motor position. In [-frame_width, +frame_width]. None if unable to find it
x_translation- rtype:
tuple | None
warning: deprecated !!!!! return True if the frames are flip through y
return y pixel size in meter
y_real_pixel_size- rtype:
float | None
y_translation- rtype:
tuple | None
z_translation- rtype:
tuple | None
- FRAME_REDUCER_CLASS#
alias of
HDF5FrameReducer
- property alignment_projections: dict | None#
dict of projections made for alignment with acquisition index as key None if not found
- Return type:
dict | None
- build_drac_metadata()#
build icat metadata dictionary filling NXtomo definition following icat definition: https://gitlab.esrf.fr/icat/hdf5-master-config/-/blob/88a975039694d5dba60e240b7bf46c22d34065a0/hdf5_cfg.xml
- Return type:
dict
- clear_cache()#
clear caches. Might be call if some data changed after first read of data or metadata
- Return type:
None
- compute_reduced_darks(reduced_method='mean', overwrite=True, output_dtype=<class 'numpy.float32'>, return_info=False)#
- Parameters:
method (ReduceMethod) – method to compute the flats
overwrite – if some flats have already been computed will overwrite them
return_info (
bool) – do we return (reduced_frames, info) or directly reduced_frames
- compute_reduced_flats(reduced_method='median', overwrite=True, output_dtype=<class 'numpy.float32'>, return_info=False)#
- Parameters:
method (ReduceMethod) – method to compute the flats
overwrite – if some flats have already been computed will overwrite them
return_info (
bool) – do we return (reduced_frames, info) or directly reduced_frames
- property darks: dict | None#
list of darks files
- Return type:
dict | None
- property detector_transformations: tuple | None#
return tuple of Transformation affecting the NXdetector
- Return type:
tuple | None
- property electric_current: list | None#
Return the sample name
- Return type:
list | None
- property energy: float | None#
energy in keV
- Return type:
float | None
- equal(other)#
:param instance to compare with :rtype:
bool:return: True if instance are equivalent- ..note:: we cannot use the __eq__ function because this object need to be
picklable
- property field_of_view#
- Returns:
field of view of the scan. None if unknown else Full or Half
- flat_field_correction(projs, proj_indexes, line=None)#
Apply flat field correction on the given data
- Parameters:
projs (Iterable) – list of projection (numpy array) to apply correction on
proj_indexes (Iterable data) – list of indexes of the projection in the acquisition sequence. Values can be int or None. If None then the index take will be the one in the middle of the flats taken.
line (int | None) – index of the line to apply flat filed. If not provided consider we want to apply flat filed on the entire frame
- Returns:
corrected data: list of numpy array
- property flat_n: int | None#
number of flat per series (computed on the first series)
- Return type:
int | None
- property flats: dict | None#
list of flats files
- Return type:
dict | None
- property frames: tuple | None#
return tuple of frames. Frames contains
- Return type:
tuple | None
- static from_identifier(identifier)#
Return the Dataset from a identifier
- get_bounding_box(axis=None)#
Return the bounding box covered by the Tomo object axis is expected to be in (0, 1, 2) or (x==0, y==1, z==2)
- Return type:
tuple
- get_identifier()#
return the dataset identifier of the scan. The identifier is insure to be unique for each scan and allow the user to store the scan as a string identifier and to retrieve it later from this single identifier.
- Return type:
- get_proj_angle_url()#
return a dictionary of all the projection. key is the angle of the projection and value is the url.
Keys are int for ‘standard’ projections and strings for return projections.
- Return type:
dict | None
- Returns:
angles as keys, radios as value.
- get_projections_intensity_monitor()#
return intensity monitor values for projections
- Return type:
dict
- get_relative_file(file_name, with_dataset_prefix=True)#
- Parameters:
file_name (str) – name of the file to create
with_dataset_prefix – If True will prefix the requested file by the dataset name like datasetname_file_name
- Return type:
str | None
- Returns:
path to the requested file according to the ‘Scan’ / ‘dataset’ location. Return none if Scan has no path
- get_sample_detector_distance(unit='m')#
- Parameters:
unit – unit requested for the distance
- Return type:
float | None
- Returns:
sample / detector distance with the requested unit
- get_sinogram(line, subsampling=1, norm_method=None, **kwargs)#
extract the sinogram from projections
- Parameters:
line – which sinogram we want
subsampling – subsampling to apply. Allows to skip some io
- Return type:
numpy.array
- Returns:
computed sinogram from projections
- static get_valid_entries(file_path)#
return the list of ‘Nxtomo’ entries at the root level
- Parameters:
file_path (
str) –- Return type:
tuple- Returns:
list of valid Nxtomo node (ordered alphabetically)
..note: entries are sorted to insure consistency
- static get_volume_output_file_name(z=None, suffix=None)#
if used by tomwer and nabu this should help for tomwer to find out the output files of anbu from a configuration file. Could help to get some normalization there
- property group_size#
if found dict of projections urls with index during acquisition as key
- property instrument_name: str | None#
- Return type:
str | None
- Returns:
instrument name
- is_abort(**kwargs)#
- Returns:
True if the acquisition has been abort
- static is_tomoscan_dir(directory, **kwargs)#
Check if the given directory is holding an acquisition
- Parameters:
directory (
str) –- Return type:
bool- Returns:
does the given directory contains any acquisition
- load_from_dict(_dict)#
Load properties contained in the dictionary.
- Parameters:
_dict (
dict) – dictionary to load- Return type:
- Returns:
self
- Raises:
ValueError if dict is invalid
- load_reduced_darks(inputs_urls=(DataUrl(valid=True, scheme='silx', file_path='{scan_prefix}_darks.hdf5', data_path='{entry}/darks/{index}', data_slice=None),), metadata_input_urls=(DataUrl(valid=True, scheme='silx', file_path='{scan_prefix}_darks.hdf5', data_path='{entry}/darks/', data_slice=None),), return_as_url=False, return_info=False)#
load reduced dark (median / mean…) into files
- Parameters:
inputs_urls (
tuple) – where to load the reduced darks. A default value is provided by the children class. You better know what you are doing if you modify the default value.metadata_input_urls – where to load the reduced darks metadata. A default value is provided by the children class. You better know what you are doing if you modify the default value.
return_as_url (
bool) – if True then instead of returning the reduced frames as 2D numpy arrays it will return them as a silx DataUrlreturn_info (
bool) – if False only return return the dict of reduced frames (frame index as key (int) and frame as a 2D numpy array or silx Data Url as value) if True then return (dict of reduced frames, darks info / metadata)
Here is an example of usage:
scan = ... # scan must be an instance of TomoScanBase like NXtomoScan() reduced_darks = scan.load_reduced_darks() reduced_darks, darks_infos = scan.load_reduced_darks(return_info=True) dark_frame_np_array = reduced_darks[0]
- Return type:
dict
- load_reduced_flats(inputs_urls=(DataUrl(valid=True, scheme='silx', file_path='{scan_prefix}_flats.hdf5', data_path='{entry}/flats/{index}', data_slice=None),), metadata_input_urls=(DataUrl(valid=True, scheme='silx', file_path='{scan_prefix}_flats.hdf5', data_path='{entry}/flats/', data_slice=None),), return_as_url=False, return_info=False)#
load reduced flats frames
- Parameters:
inputs_urls (
tuple) – where to load the reduced flats. A default value is provided by the children class. You better know what you are doing if you modify the default value.metadata_input_urls – where to load the reduced flats metadata. A default value is provided by the children class. You better know what you are doing if you modify the default value.
return_as_url (
bool) – if True then instead of returning the reduced frames as 2D numpy arrays it will return them as a silx DataUrlreturn_info (
bool) – if False only return return the dict of reduced frames (frame index as key (int) and frame as a 2D numpy array or silx Data Url as value) if True then return (dict of reduced frames, flats info / metadata)
Here is an example of usage:
scan = ... # scan must be an instance of TomoScanBase like NXtomoScan() reduced_flats = scan.load_reduced_flats() reduced_flats, flats_infos = scan.load_reduced_flats(return_info=True)
- Return type:
dict
- property magnification#
number of projection WITHOUT the return projections
- static map_urls_on_scan_range(urls, n_projection, scan_range)#
map given urls to an angle regarding scan_range and number of projection. We take the hypothesis that ‘extra projection’ are taken regarding the ‘id19’ policy:
If the acquisition has a scan range of 360 then:
if 4 extra projection, the angles are (270, 180, 90, 0)
if 5 extra projection, the angles are (360, 270, 180, 90, 0)
If the acquisition has a scan range of 180 then:
if 2 extra projections: the angles are (90, 0)
if 3 extra projections: the angles are (180, 90, 0)
..warning:: each url should contain only one radio.
- Parameters:
urls – dict with all the urls. First url should be the first radio acquire, last url should match the last radio acquire.
n_projection – number of projection for the sample.
scan_range – acquisition range (usually 180 or 360)
- Return type:
dict- Returns:
angle in degree as key and url as value
- Raises:
ValueError if the number of extra images found and scan_range are incoherent
- static node_is_nxtomo(node)#
check if the given h5py node is an nxtomo node or not
- Return type:
bool
- property path: str | None#
- Return type:
str | None
- Returns:
path of the scan root folder.
- property pixel_size: float | None#
return x pixel size in meter
- Return type:
float | None
- property projections: dict | None#
if found dict of projections urls with index during acquisition as key
- Return type:
dict | None
- property projections_compacted#
Return a compacted view of projection frames.
- Returns:
Dictionary where the key is a list of indices, and the value is the corresponding silx.io.url.DataUrl with merged data_slice
- property sample_detector_distance: float | None#
return sample detector distance in meter
- Return type:
float | None
- property sample_name#
if found dict of projections urls with index during acquisition as key
- save_reduced_darks(darks, output_urls=(DataUrl(valid=True, scheme='silx', file_path='{scan_prefix}_darks.hdf5', data_path='{entry}/darks/{index}', data_slice=None),), darks_infos=None, metadata_output_urls=(DataUrl(valid=True, scheme='silx', file_path='{scan_prefix}_darks.hdf5', data_path='{entry}/darks/', data_slice=None),), overwrite=False)#
Dump computed dark (median / mean…) into files.
- Parameters:
darks (
dict) – dictionary with frame indices as key (int) and a 2D numpy array as value.output_urls (
tuple) – tuple of silx DataUrl, where to save the darks. Default value is usually provided by children class directly. You better know what you are doing if you modify the default value.darks_infos – information regarding darks (metadata) like the machine electric current, exposure time…
metadata_output_urls – tuple of silx DataUrl, where to save the metadata / darks information. Default value is usually provided by children class directly You better know what you are doing if you modify the default value.
overwrtie – if the output files exist then will overwrite them.
Here is an example on how to save your own reduced dark / flat
from tomoscan.framereducer.reducedframesinfos import ReducedFramesInfos ... scan = ... # scan must be an instance of TomoScanBase like NXtomoScan() darks_infos.count_time = [2.5] darks_infos.machine_electric_current = [13.1] scan.save_reduced_darks( darks={ 0: dark_frame, # dark_frame is a 2d numpy array }, darks_infos=darks_infos, overwrite=True, )
- save_reduced_flats(flats, output_urls=(DataUrl(valid=True, scheme='silx', file_path='{scan_prefix}_flats.hdf5', data_path='{entry}/flats/{index}', data_slice=None),), flats_infos=None, metadata_output_urls=(DataUrl(valid=True, scheme='silx', file_path='{scan_prefix}_flats.hdf5', data_path='{entry}/flats/', data_slice=None),), overwrite=False)#
Dump computed dark (median / mean…) into files.
- Parameters:
flats (
dict) – dictionary with frame indices as key (int) and a 2D numpy array as value.output_urls (
tuple) – tuple of silx DataUrl, where to save the flats. Default value is usually provided by children class directly. You better know what you are doing if you modify the default value.flats_infos – information regarding flats (metadata) like the machine electric current, exposure time…
metadata_output_urls (
tuple) – tuple of silx DataUrl, where to save the metadata / flats information. Default value is usually provided by children class directly You better know what you are doing if you modify the default value.overwrite (
bool) – if the output files exist then will overwrite them.
Here is an example on how to save your own reduced dark / flat
from tomoscan.framereducer.reducedframesinfos import ReducedFramesInfos ... scan = ... # scan must be an instance of TomoScanBase like NXtomoScan() flats_infos = ReducedFramesInfos() flats_infos.count_time = [2.5, 1.2] flats_infos.machine_electric_current = [12.5, 13.1] # for normalization the first reduced flat (at index 1) will have 2.5 as count time and 12.5 as machine electric current # the second reduced flat frame (at index 1002) will have 1.2 as count time and 13.1 as machine electric current scan.save_reduced_darks( darks={ 1: flat_frame_1, # flat_frame_1 is a 2d numpy array 1002: flat_frame_2, # flat_frame_2 is another 2d numpy array }, flats_infos=flats_infos, overwrite=True, )
- Return type:
dict
- property sequence_name#
Return the sequence name
- set_check_behavior(run_check=True, raise_error=False, log_level=30)#
when user require to access to scan frames NXtomoScan build them (frames property). Some check can be made during this stage to know if the scan has some broken virtual-dataset (vds) or if the vds is linked to more file than the system might handle.
In this case the ‘vds-check’ can either raise an error or log potential issues with a specific log level
- property source_sample_distance: float | None#
- Return type:
float | None
- Returns:
source / sample distance (in meter). Expected to be negative (NXtomo convention).
- property splitted_flat_series: dict | None#
split flat according to flat indices
- Return type:
dict | None
- to_dict()#
- Return type:
dict- Returns:
convert the TomoScanBase object to a dictionary. Used to serialize the object for example.
- property tomo_n: int | None#
number of projection WITHOUT the return projections
- Return type:
int | None
- property type: str#
- Return type:
str- Returns:
type of the scanBase (can be ‘edf’ or ‘hdf5’ for now).
- update()#
Parse the root folder and files to update information
- Return type:
None
- property x_flipped: bool#
warning: deprecated !!!!! return True if the frames are flip through x
- Return type:
bool
- property x_pixel_size: float | None#
return x pixel size in meter
- Return type:
float | None
- property x_rotation_axis_pixel_position#
- Returns:
Estimated center of rotation estimated from motor position. In [-frame_width, +frame_width]. None if unable to find it
- property y_flipped: bool#
warning: deprecated !!!!! return True if the frames are flip through y
- Return type:
bool
- property y_pixel_size: float | None#
return y pixel size in meter
- Return type:
float | None